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Relativistic Rotation of the Rigid Body in the Rodrigues – Hamilton Parameters: Lagrange Function and Equations of Motion Cover

Relativistic Rotation of the Rigid Body in the Rodrigues – Hamilton Parameters: Lagrange Function and Equations of Motion

Open Access
|Sep 2018

References

  1. Suslov G.K. (1946): Theoretical mechanics. OGIZ, Moscow, (in Russian).
  2. MacMillan W.D. (1936): Dynamics of rigid bodies, New Yotk and London.
  3. Landau L.D. and Lifshitz E.M. (1967): The Classical Theory of Fields, Moscow: "Nauka". (in Russian)10.1016/B978-0-08-009106-8.50005-4
  4. Eroshkin G.I., Pashkevich V.V. (1997): Numerical simulation of the rotation motion of the Earth and Moon, Dynamics and Astrometry of Natural and Artificial Celestial Bodies, Proceedings of IAU Colloquium 165 (I.M. Wytrzyszczak, J.H. Lieske, R.A. Feldman eds.), Kluwer, Dordrecht, pp. 275-281.10.1007/978-94-011-5534-2_37
  5. Pashkevich V.V. (2000): Construction of the High-Precision Numerical Theory of the Rigid Earth Rotation, Artificial Satellites, Journal of Planetary Geodesy, Vol. 35, No 2, pp. 59-71.
DOI: https://doi.org/10.2478/arsa-2018-0008 | Journal eISSN: 2083-6104 | Journal ISSN: 1509-3859
Language: English
Page range: 89 - 115
Submitted on: Jan 2, 2018
Accepted on: Sep 3, 2018
Published on: Sep 25, 2018
Published by: Polish Academy of Sciences, Space Research Centre
In partnership with: Paradigm Publishing Services
Publication frequency: 4 issues per year

© 2018 V.V. Pashkevich, G.I. Eroshkin, published by Polish Academy of Sciences, Space Research Centre
This work is licensed under the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 License.